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Energy-dependent X-ray polarization from magnetar 4U 0142+61

Contribution grade

Astrophysics · Source-reported experimental result or reusable measurement method

Reference score100,000Provisional editorial estimate of this exact contribution; its grade is assessed separately.

What changed

Taverna and colleagues used IXPE to measure phase-averaged X-ray polarization from magnetar 4U 0142+61. They found about 12 ± 1% across 2–8 keV, with different polarization behavior at lower and higher energies and an approximately 90-degree angle change across the intervening band.

Scientific scope

Taverna and colleagues used IXPE to measure phase-averaged X-ray polarization from magnetar 4U 0142+61. They found about 12 ± 1% across 2–8 keV, with different polarization behavior at lower and higher energies and an approximately 90-degree angle change across the intervening band. The observed polarization is not an unambiguous direct detection of QED vacuum birefringence: the authors explicitly state that the energy- and phase-integrated polarization is insufficient to establish that effect alone. Their surface, atmosphere and magnetospheric scenarios are model-dependent and not unique; geometric angles are poorly constrained. The 4–5 keV polarization lies below instrumental sensitivity, so the angle there is poorly determined. Alternative processing analyzes the same IXPE observation and is not independent replication. The supplement describes normally distributed Stokes parameters as correlated in one sentence and uncorrelated in another; this literal inconsistency needs source-version and calculation reconciliation rather than silent correction. The individual contributor list shown here is incomplete.

Evidence

The linked original works support the scoped statement and contribution attribution. WRS has not independently replayed experiments or reconstructed a full mathematical proof. The observed polarization is not an unambiguous direct detection of QED vacuum birefringence: the authors explicitly state that the energy- and phase-integrated polarization is insufficient to establish that effect alone. Their surface, atmosphere and magnetospheric scenarios are model-dependent and not unique; geometric angles are poorly constrained. The 4–5 keV polarization lies below instrumental sensitivity, so the angle there is poorly determined. Alternative processing analyzes the same IXPE observation and is not independent replication. The supplement describes normally distributed Stokes parameters as correlated in one sentence and uncorrelated in another; this literal inconsistency needs source-version and calculation reconciliation rather than silent correction. The individual contributor list shown here is incomplete.

Contributors

Provisional WRS assessment, edition 2026-10-28.1. Independent expert calibration is pending. This grade does not certify correctness or assign ownership.

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